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Induced Gravitational Collapse in the BATSE era: the case of GRB 970828
R. Ruffini, Jorge A. Rueda, C. Barbarino +8
Following the recently established "Binary-driven HyperNova" (BdHN) paradigm, we here interpret GRB 970828 in terms of the four episodes typical of such a model. The "Episode 1", u…
On a novel distance indicator for Gamma-Ray Bursts associated with Supernovae
Giovanni Battista Pisani, Luca Izzo, Remo Ruffini +5
It has been proposed that the temporal coincidence of a gamma-ray burst (GRB) and a type Ib/c supernova (SN) can be explained with the concept of induced gravitational collapse (IG…
A white dwarf merger as progenitor of the anomalous X-ray pulsar 4U 0142+61?
J. A. Rueda, K. Boshkayev, L. Izzo +5
It has been recently proposed that massive fast-rotating highly-magnetized white dwarfs could describe the observational properties of some of Soft Gamma-Ray Repeaters (SGRs) and A…
GRB 090510: a disguised short GRB with the highest Lorentz factor and circumburst medium
M. Muccino, R. Ruffini, C. L. Bianco +3
GRB 090510, observed both by Fermi and AGILE satellites, is the first bright short-hard Gamma-Ray Burst (GRB) with an emission from the keV up to the GeV energy range. Within the F…
SGR 0418+5729, Swift J1822.3-1606, and 1E 2259+586 as massive fast rotating highly magnetized white dwarfs
K. Boshkayev, L. Izzo, Jorge A. Rueda +1
Following Malheiro et al. (2012) we describe the so-called low magnetic field magnetars, SGR 0418+5729, Swift J1822.3--1606, as well as the AXP prototype 1E 2259+586 as massive fas…
Novel distance indicator for gamma-ray bursts associated with supernovae
G. B. Pisani, L. Izzo, R. Ruffini +5
Context. It has been proposed that the temporal coincidence of a gamma-ray burst (GRB) and a type Ib/c supernova (SN) can be explained with the concept of induced gravitational col…